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Helium Abundance in the Most Metal‐deficient Blue Compact Galaxies: I Zw 18 and SBS 0335−052

  • Authors: Yuri I. Izotov, Frederic H. Chaffee, Craig B. Foltz, Richard F. Green, Natalia G. Guseva, and Trinh X. Thuan

Izotov et al. 1999 The Astrophysical Journal 527 757.

  • Provider: AAS Journals

Caption: Fig. 10.

Joint fits to the baryon‐to‐photon number ratio, ﹩\mathrm{log}\,\eta _{10}﹩, and the equivalent number of light neutrino species ﹩N_{\nu }﹩ using a χ2 analysis with the code developed by Fiorentini et al. (1998) and Lisi et al. (1999) (a) for primordial abundance values ﹩Y_{p}﹩ (this paper), (D/H)p (Burles & Tytler 1998b), and (7Li/H)p (Bonifacio & Molaro 1997) and (b) for best choice of primordial abundance values ﹩Y_{p}﹩ (this paper), (D/H)p (Levshakov et al. 1999), and (7Li/H)p (Vauclair & Charbonnel 1998). The minimum value ﹩\chi ^{2}_{\mathrm{min}\,}=0.001﹩ in the latter case is achieved for ﹩\mathrm{log}\,\eta _{10}=0.648﹩ (﹩\eta =4.45\times 10^{-10}﹩) and ﹩N_{\nu }=3.006﹩ (filled circle). Thin and thick solid lines are 1 σ and 2 σ deviations, respectively. The experimental value ﹩N_{\nu }=2.993﹩ (Caso et al. 1998) is shown by dashed line.

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